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Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany. sierks@mps.mpg.de
Images obtained by the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) cameras onboard the Rosetta spacecraft reveal that asteroid 21 Lutetia has a complex geology and one of the highest asteroid densities measured so far, 3.4 ± 0.3 grams per cubic centimeter. The north pole region is covered by a thick layer of regolith, which is seen to flow in major landslides associated with albedo variation. Its geologically complex surface, ancient surface age, and high density suggest that Lutetia is most likely a primordial planetesimal. This contrasts with smaller asteroids visited by previous spacecraft, which are probably shattered bodies, fragments of larger parents, or reaccumulated rubble piles.
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Direct Access Service, Old Sandy Rd Clinic, Glasgow, Scotland, UK.
Objective: This study was designed to examine the existence of deficits in mentalizing or theory of mind (ToM) in children with traumatic brain injury (TBI).Research design: ToM functioning was assessed in 12 children aged 6-12 years with TBI and documented frontal lobe damage and compared to 12 controls matched for age, sex and verbal ability. Brief measures of attention and memory were also included.Main outcome and results: The TBI group was significantly impaired relative to controls on the advanced ToM measure and a measure of basic emotion recognition. No difference was found in a basic measure of ToM.Conclusion: Traumatic brain damage in childhood may disrupt the developmental acquisition of emotion recognition and advanced ToM skills. The clinical and theoretical importance of these findings is discussed and the implications for the assessment and treatment of children who have experienced TBI are outlined.
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PLANET/RoboNet Collaboration, CNRS, Université Pierre et Marie Curie UMR7095, 98bis Boulevard Arago, 75014 Paris, France. beaulieu@iap.fr
In the favoured core-accretion model of formation of planetary systems, solid planetesimals accumulate to build up planetary cores, which then accrete nebular gas if they are sufficiently massive. Around M-dwarf stars (the most common stars in our Galaxy), this model favours the formation of Earth-mass (M(o)) to Neptune-mass planets with orbital radii of 1 to 10 astronomical units (au), which is consistent with the small number of gas giant planets known to orbit M-dwarf host stars. More than 170 extrasolar planets have been discovered with a wide range of masses and orbital periods, but planets of Neptune's mass or less have not hitherto been detected at separations of more than 0.15 au from normal stars. Here we report the discovery of a 5.5(+5.5)(-2.7) M(o) planetary companion at a separation of 2.6+1.5-0.6 au from a 0.22+0.21-0.11 M(o) M-dwarf star, where M(o) refers to a solar mass.(We propose to name it OGLE-2005-BLG-390Lb, indicating a planetary mass companion to the lens star of the microlensing event.) The mass is lower than that of GJ876d (ref. 5), although the error bars overlap. Our detection suggests that such cool, sub-Neptune-mass planets may be more common than gas giant planets, as predicted by the core accretion theory.
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1James Graham Brown Cancer Center, University of Louisville School of Medicine, Louisville, KY, USA.
E1B55K-deleted dl1520 could selectively replicate in cancer cells and has been used in clinical trials as an antitumor agent. The mechanism of virus selective replication in cancer cells, including a possible role of p53, is unclear. Studies with established cancer cell lines have demonstrated that some cancer cells are resistant to dl1520 replication, regardless of the p53 status. Hep3B cells supported the E1b-deleted adenoviruses to replicate, whereas Saos2 cells were resistant to viral replication. We applied p53-null Hep3B and Saos2 cells as models to clarify the replication ability of E1B55K-deleted adenoviruses with different expression levels of E1a. We show that lower E1A expression in Saos2 may be the reason for the poor replication in some cancer cells due to the fact that E1a promoter was less activated in Saos2 than in Hep3B. We also demonstrate that the E1B55K protein can increase E1A expression in Saos2 cells for efficient virus replication. In addition, the upstream regions of the E1a promoter have transcriptional activity in Hep3B cells but not in Saos2 cells. The viral E1B55K protein may activate cancer cellular factor(s) that targets the upstream regions of the E1a gene to increase its expression. This is the first study demonstrating that E1B55K protein affects the E1A production levels that is related to cancer selective replication. Our studies have suggested that increase of E1A expression from E1b-deleted adenoviruses may enhance killing cancer cells that otherwise are resistant to viral replication.Cancer Gene Therapy advance online publication, 9 December 2005; doi:10.1038/sj.cgt.7700923.
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James Graham Brown Cancer Center, University of Louisville School of Medicine, Louisville, Kentucky, USA.
One of the promising strategies for targeting replication of oncolytic adenovirus in tumor cells is to regulate the expression of essential viral genes such as E1a by using tumor- or tissue-specific promoters that are preferentially active in cancer cells. However, this approach may lead to some degree of viral replication in normal cells other than in cancer cells if the viral gene also expresses in normal cells. In this study, we investigated the effect of E1a expression levels on the virus replication ability in human cells. Three vectors, all with mutated E1B55K, were created, one without any promoter controlling the E1a gene and two vectors with the E1a gene being controlled by either its endogenous promoter or a strong CMV promoter. We observed that the CMV promoter-mediated high levels of E1A expression could increase virus replication, resulting in the titers of the E1B55K-mutated virus being even higher than the wild-type virus in some cancer cells. However, the strong CMV promoter could not always enhance virus replication, such as in cancer cells OE33 and OsACL. The results suggest that whether increased E1A levels would enhance E1B55K-mutated virus replication may be also depended on cellular factors or pathways in cancer cells. We also observed that the virus without any promoter for the E1a gene could still express leaky levels of E1A which can lead to viral replication in normal and cancer cells. Future efforts in the development of transcription-controlled oncolytic adenoviruses should focus on how to completely block E1a expression in normal cells.
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[My paper] K J Meech, N Ageorges, M F A'Hearn, C Arpigny, A Ates, J Aycock, S Bagnulo, J Bailey, R Barber, L Barrera, R Barrena, J M Bauer, M J S Belton, F Bensch, B Bhattacharya, N Biver, G Blake, D Bockelée-Morvan, H Boehnhardt, B P Bonev, T Bonev, M W Buie, M G Burton, H M Butner, R Cabanac, R Campbell, H Campins, M T Capria, T Carroll, F Chaffee, S B Charnley, R Cleis, A Coates, A Cochran, P Colom, A Conrad, I M Coulson, J Crovisier, J deBuizer, R Dekany, J de Léon, N Dello Russo, A Delsanti, M DiSanti, J Drummond, L Dundon, P B Etzel, T L Farnham, P Feldman, Y R Fernández, M D Filipovic, S Fisher, A Fitzsimmons, D Fong, R Fugate, H Fujiwara, T Fujiyoshi, R Furusho, T Fuse, E Gibb, O Groussin, S Gulkis, M Gurwell, E Hadamcik, O Hainaut, D Harker, D Harrington, M Harwit, S Hasegawa, C W Hergenrother, P Hirst, K Hodapp, M Honda, E S Howell, D Hutsemékers, D Iono, W-H Ip, W Jackson, E Jehin, Z J Jiang, G H Jones, P A Jones, T Kadono, U W Kamath, H U Käufl, T Kasuga, H Kawakita, M S Kelley, F Kerber, M Kidger, D Kinoshita, M Knight, L Lara, S M Larson, S Lederer, C-F Lee, A C Levasseur-Regourd, J Y Li, Q-S Li, J Licandro, Z-Y Lin, C M Lisse, G LoCurto, A J Lovell, S C Lowry, J Lyke, D Lynch, J Ma, K Magee-Sauer, G Maheswar, J Manfroid, O Marco, P Martin, G Melnick, S Miller, T Miyata, G H Moriarty-Schieven, N Moskovitz, B E A Mueller, M J Mumma, S Muneer, D A Neufeld, T Ootsubo, D Osip, S K Pandea, E Pantin, R Paterno-Mahler, B Patten, B E Penprase, A Peck, G Petitas, N Pinilla-Alonso, J Pittichova, E Pompei, T P Prabhu, C Qi, R Rao, H Rauer, H Reitsema, S D Rodgers, P Rodriguez, R Ruane, G Ruch, W Rujopakarn, D K Sahu, S Sako, I Sakon, N Samarasinha, J M Sarkissian, I Saviane, M Schirmer, P Schultz, R Schulz, P Seitzer, T Sekiguchi, F Selman, M Serra-Ricart, R Sharp, R L Snell, C Snodgrass, T Stallard, G Stecklein, C Sterken, J A Stüwe, S Sugita, M Sumner, N Suntzeff, R Swaters, S Takakuwa, N Takato, J Thomas-Osip, E Thompson, A T Tokunaga, G P Tozzi, H Tran, M Troy, C Trujillo, J Van Cleve, R Vasundhara, R Vazquez, F Vilas, G Villanueva, K von Braun, P Vora, R J Wainscoat, K Walsh, J Watanabe, H A Weaver, W Weaver, M Weiler, P R Weissman, W F Welsh, D Wilner, S Wolk, M Womack, D Wooden, L M Woodney, C Woodward, Z-Y Wu, J-H Wu, T Yamashita, B Yang, Y-B Yang, S Yokogawa, A C Zook, A Zauderer, X Zhao, X Zhou, J-M Zucconi
Institute for Astronomy, University of Hawaii at Manoa, 2680 Woodlawn Drive, Honolulu, HI 96822, USA.
On 4 July 2005, many observatories around the world and in space observed the collision of Deep Impact with comet 9P/Tempel 1 or its aftermath. This was an unprecedented coordinated observational campaign. These data show that (i) there was new material after impact that was compositionally different from that seen before impact;(ii) the ratio of dust mass to gas mass in the ejecta was much larger than before impact;(iii) the new activity did not last more than a few days, and by 9 July the comet's behavior was indistinguishable from its pre-impact behavior; and (iv) there were interesting transient phenomena that may be correlated with cratering physics.
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Department of Obstetrics, Newcastle upon Tyne, United Kingdom.
OBJECTIVE: To determine the relation between the obstetric management of fetal distress and cerebral palsy. METHODS: The obstetric details of all 78 children with cerebral palsy born in a geographically defined area between 1975-1980 were compared with those of 591 control children. RESULTS: Fetal distress was identified more frequently in children with cerebral palsy who were born at term (24%) than among controls (11%). There was an inappropriate response to fetal distress in 12% of children with cerebral palsy but in only 3% of controls. CONCLUSIONS: If fetal distress in some way causes subsequent cerebral palsy, then the data in this study suggest that its complete elimination might be expected to reduce the birth prevalence of cerebral palsy by 15.6%."Perfect" obstetric management of fetal distress might reduce the birth prevalence of cerebral palsy by 9% in term infants or 6% overall.
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Fully refined, bleached, deodorized corn oil and soy oil, and lightly hydrogenated, winterized soy oil were compared for effectiveness in lowering plasma cholesterol. Twenty-four, healthy, young college students were the subjects for the 10-wk studies. At the 300 cal level, the corn oil and unhydrogenated soy oil diets contained approximately 53 g of polyunsaturated and 26 g of saturated fat. The hydrogenated soy oil diet contained 42 and 25 g, respectively. All diets contained approximately 700 mg of cholesterol. Corn oil and unhydrogenated soy oil were equally effective in lowering both total and low density lipoprotein cholesterol. Lightly hydrogenated soy oil was also quite effective, but less so that the more unsaturated oils. Triglycerides were also lowered, but very low density and high density lipoprotein cholesterol concentrations, as well as total high density lipoproteins, were scarcely affected. All of the polyunsaturated fat diets produced small but statistically significant reductions in the cholesterol to protein ratio of all three lipoproteins.
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2012-05-23 18:28:17 © BioInfoBank Institute